Simulations indicate that order-of-magnitude changes in TiO2 and SiO2 abundances in lava melts produce distinguishable TiO, SiO, and SiO2 features in dry lava planet emission spectra, potentially observable with 12 JWST eclipses for the brightest targets.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
UNVERDICTED 2representative citing papers
Top-heavy thermochemical geodynamo simulations show heterogeneous outer boundary heat flux reproduces observed longitudinal inclination anomaly variations, while elevated chemical driving reduces longitudinal structures and promotes polar radial field minima.
citing papers explorer
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Sensitivity of Dry Lava Planet Atmospheric Emission Spectra to Changes in Lava Compositions
Simulations indicate that order-of-magnitude changes in TiO2 and SiO2 abundances in lava melts produce distinguishable TiO, SiO, and SiO2 features in dry lava planet emission spectra, potentially observable with 12 JWST eclipses for the brightest targets.
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Paleomagnetic signatures of core-mantle interactions inferred from top-heavy thermochemical geodynamo simulations
Top-heavy thermochemical geodynamo simulations show heterogeneous outer boundary heat flux reproduces observed longitudinal inclination anomaly variations, while elevated chemical driving reduces longitudinal structures and promotes polar radial field minima.